The time it takes for a Cepheid star to go from it's brightest, to it's dimmest, and back to it's brightest again. =] Hope that helped.
Cepheid variables are high-mass, pulsating variables exhibiting a regular relationship between the period of pulsation and luminosity. When a star's evolutionary track carries it through a region called the instability strip in the HR diagram, the star becomes unstable and begins to pulsate. These stars are important to astronomers who study galaxies because Cepheids can be seen at extragalactic distances, and their period or pulsation tells us their luminosities, which in turn tells us their distances. - Cincinnati
A Cepheid is a member of a particular class of variable stars. The relationship between a Cepheid variable's luminosity and pulsation period is quite precise, securing classical Cepheids as viable standard candles and the foundation of the Extragalactic Distance Scale. See related link for more information
A cepheid phase is when a star starts expand and contract and it loses its outer layers in the process.at least that's what i was told.
binary star
She discovered the period luminosity relationship of cepheid variables
A Cepheid is a member of a class of pulsating variable stars. The relationship between a Cepheid variable's luminosity and pulsation period is quite precise, securing Cepheids as viable standard candles and the foundation of the Extragalactic Distance Scale.
Cepheid variables are high-mass, pulsating variables exhibiting a regular relationship between the period of pulsation and luminosity. When a star's evolutionary track carries it through a region called the instability strip in the HR diagram, the star becomes unstable and begins to pulsate. These stars are important to astronomers who study galaxies because Cepheids can be seen at extragalactic distances, and their period or pulsation tells us their luminosities, which in turn tells us their distances. - Cincinnati
A Cepheid is a member of a particular class of variable stars. The relationship between a Cepheid variable's luminosity and pulsation period is quite precise, securing classical Cepheids as viable standard candles and the foundation of the Extragalactic Distance Scale. See related link for more information
RR Lyrae stars. (Sometimes these stars are classed as a type of "Cepheid variable", but they are usually considered as a separate star type.)
A cepheid phase is when a star starts expand and contract and it loses its outer layers in the process.at least that's what i was told.
There are many ways to calculate distance at huge scales. One popular way is using a Cepheid within the nebula. A Cepheid is a very luminous variable star (a star that changes brightness). The changing of brightness tells us a lot about the distance by measuring the period (time) and the luminosity. See the related link for more methods.
It really depends on the type of star, but for certain star types, there is a relationship between the period and the absolute brightness, so if the period is observed, the absolute brightness can be deduced. Yes. It seems like this question is about the Cepheid variables.
binary star
The general name is a 'Pulsar'. The reason for the pulsation may differ depending on the star system.
She discovered the period luminosity relationship of cepheid variables
The main star of the system is Ursa Minor Aa which is a Cepheid Variable. Its apparent magnitude averages at 1.98
The apparent brightness of the main star in the system is 1.98 but remember that this is a Cepheid variable.